0
Assigned ID: 509
----- Attempting Submission 1 (Fri Apr 11 14:54:47 GMT 2014) -----
POS TARG & PATTERN should be used carefully with ACS ramp or WFC3 quad filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp or WFC3 quad filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp or WFC3 quad filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp or WFC3 quad filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp or WFC3 quad filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp or WFC3 quad filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp or WFC3 quad filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp or WFC3 quad filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp or WFC3 quad filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp or WFC3 quad filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp or WFC3 quad filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp or WFC3 quad filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp or WFC3 quad filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp or WFC3 quad filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp or WFC3 quad filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp or WFC3 quad filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp or WFC3 quad filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp or WFC3 quad filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp or WFC3 quad filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp or WFC3 quad filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp or WFC3 quad filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp or WFC3 quad filters as central wavelengths & transmission efficiencies vary within the apertures.
0
----- Attempting Submission 4 (Thu Nov 06 18:13:56 GMT 2014) -----
----- Attempting Submission 5 (Thu Dec 11 19:36:09 GMT 2014) -----
----- Attempting Submission 6 (Wed Dec 31 20:23:17 GMT 2014) -----
----- Attempting Submission 7 (Tue Feb 03 21:49:20 GMT 2015) -----
----- Attempting Submission 8 (Wed Apr 08 00:55:37 GMT 2015) -----
----- Attempting Submission 9 (Mon Jun 01 19:55:08 GMT 2015) -----
----- Attempting Submission 10 (Fri Jul 24 17:16:16 GMT 2015) -----
we increased acq time for visit 12, (based on experience with visit 20), adjusted G430M exptimes
accordingly and ran the Orbit and Visit planners for them.
Do QSO2s have Narrow Line Region Outflows? Implications for quasar-mode feedback
The correlation between the masses of galaxy bulges and the super-massive
black holes (BH) at their gravitational centers suggests that they co-evolve.
The process thought to regulate bulge/BH growth is ``AGN feedback'', either in
the form of radiation-driven (``quasar mode'') or mechanically driven (e.g.,
``radio mode'') outflows. Studies of Seyfert galaxies have revealed massive
gas flows through the Narrow Line Region (NLR), likely radiatively driven by
the AGN. Although one might naively expect that the magnitude of these outflows
would scale with luminosity, a recent ground-based study of the NLR of QSO2s
suggests more chaotic kinematics, with little evidence for grand-scale outflows.
Are the outflows disrupted close to the AGN? If so, it casts doubt on the
effectiveness of quasar-mode feedback. However, based on what is observed in
Seyferts and scaling with luminosity, the outflow-dominated regions in QSO2s
should be ~ 1 kpc, which cannot be resolved in ground-based optical spectra.
Therefore, we propose to obtain HST/ACS images and STIS long-slit spectra
of 11 radio-quiet QSO2s, selected from the Reyes et al. (2008) sample. With
these data, we will measure and model the NLR kinematics, probe the dynamics
of the gas, and, ultimately, determine whether AGN-driven outflows exist in
QSO2s. These results will have profound implications towards our understanding
of AGN feedback.
Although AGN-driven outflows appear to be common in the Narrow Line Regions (NLRs) of Seyfert galaxies, which suggests their importance in AGN feedback, ground based studies of the NLRs of QSO2s indicate more chaotic kinematics. If AGN-driven ouflows do not scale with luminosity, it casts doubt on the effiency of quasar-mode feedback as a mechanism for quenching star-formation. However, it requires HST resolution to determine whether NLR outflows are present in QSO2s. To that end, we will obtain ACS/[OIII] images and STIS long slit/G430M spectra of 11 radio-quiet QSO2s from the sample of Reyes et al (2008). The [OIII] images will be used to map the extent and morphology of the NLR and will, therefore, be used to determine the alignment for the STIS specta. The spectra will be used to map the kinematics at the sub-kpc scale, which will reveal whether outflows are present. The scheduling of the STIS spectra must be constrained In order to allow time to analyze the ACS images and, thus, decide on the slit alignments.
CALIBRATION ORBITS: As per STScI policy, 36 internal orbits have been added to this proposal for the purpose of obtaining subarray bias frames that are contemporaneous with the science observations. These internal orbits will be charged to STScI's Cycle 22 ACS Calibration Program, not to GO 13728. The ACS Instrument Team at STScI is responsible for producing superbias reference files from the bias frames obtained in this GO proposal.
AGN/QUASARS
12
false
false
false
false
SUPPORTED
GALAXY
NLR
QUASAR
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
NLR
QUASAR
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
NLR
QUASAR
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
NLR
QUASAR
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
NLR
QUASAR
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
NLR
QUASAR
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
NLR
QUASAR
This object was generated by the targetselector and retrieved from the NED database.
J2000
J2000
GALAXY
NLR
QUASAR
This object was generated by the targetselector and retrieved from the NED database.
J2000
J2000
GALAXY
NLR
QUASAR
This object was generated by the targetselector and retrieved from the NED database.
J2000
J2000
GALAXY
NLR
QUASAR
This object was generated by the targetselector and retrieved from the NED database.
J2000
J2000
GALAXY
NLR
QUASAR
This object was generated by the targetselector and retrieved from the NED database.
J2000
J2000
ACS/WFC
RampFilter
No
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FR505N
ACS/WFC
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No
FR647M
STIS/CCD
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G430M
5216
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No
No
FR551N
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FR647M
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G430M
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ACS/WFC
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G750M
5734
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ACS/WFC
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FR647M
STIS/CCD
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G430M
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ACS/WFC
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FR647M
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FR551N
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FR647M
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G430M
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ACS/WFC
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FR551N
ACS/WFC
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No
No
FR647M
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No
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G430M
5471
ACS/WFC
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No
No
FR551N
ACS/WFC
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No
No
FR647M
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No
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G430M
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ACS/WFC
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No
No
FR551N
ACS/WFC
RampFilter
No
No
FR647M
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Spectroscopic
No
No
G430M
5471
ACS/WFC
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No
No
FR551N
ACS/WFC
RampFilter
No
No
FR647M
STIS/CCD
Spectroscopic
No
No
G430M
5471
ACS/WFC
RampFilter
No
No
FR551N
ACS/WFC
RampFilter
No
No
FR647M
STIS/CCD
Spectroscopic
No
No
G430M
5471
POS-TARG
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ACS-WFC-DITHER-LINE
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POS-TARG
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3
90.0
STIS-ALONG-SLIT
2
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The scheduling data was generated by CASM 22.2.
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